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arXiv · astro-ph/0103275

TeV Neutrinos from Successful and Choked Gamma-Ray Bursts

P. Meszaros·E. Waxman
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Abstract

Core collapse of massive stars resulting in a relativistic fireball jet which breaks through the stellar envelope is a widely discussed scenario for gamma-ray burst production. For very extended or slow rotating stars, the fireball may be unable to break through the envelope. Both penetrating and choked jets will produce, by photo-meson interactions of accelerated protons, a burst of neutrinos with energies in excess of 5 TeV while propagating in the envelope. The predicted flux, from both penetrating and chocked fireballs, should be easily detectable by planned cubic kilometer neutrino telescopes.

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P. Meszaros, E. Waxman. 2001-09-11. TeV Neutrinos from Successful and Choked Gamma-Ray Bursts. https://doi.org/10.1103/physrevlett.87.171102

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